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Icy Volcanoes Likely Shape Saturn's Smooth Moon
05/01/2007
From Space.com
By David Powell
(Additional comments below)
Saturn's icy moon Dione may have much in
common with its active sibling Enceladus, new research using Cassini
spacecraft data has revealed.
Paul Schenk of the Lunar and Planetary Institute and Jeff Moore of
NASA's Ames Research Center modelled Dione's surface using digital
elevation models (DEMs). Their results indicate volcanism has been a
major force in shaping Dione's surface.
"We don't see giant shield volcanoes belching lavas," says Schenk.
"Instead we see smooth plains with low crater densities."
These plains are the hallmark of cryovolcanism, which manifests
itself as an outpouring of icy liquids from a moon's interior.
How it works
The DEMs used by Schenk and Moore reveal Dione's cryovolcanic plains
to be higher than the surrounding terrain, suggesting they may have
been emplaced in a high viscosity flow similar to terrestrial
glaciers sometime within the last 2 billion to 4 billion years.
Cryovolcanism requires a heat source to drive liquids to the
surface. At present the mechanism for this heat engine is not fully
understood but the two leading contenders are radioactive decay and
gravitational flexing.
"As far as the source of the heat, well that's the big question. It
is clear that some of the craters (on Dione) have been severely
modified by high heat flow, not unlike parts of Enceladus. Perhaps
these satellites (Dione and Enceladus) were very hot to begin with
and had continued tidal heating to keep them warm," Schenk told
SPACE.com.
This tidal heating of these moons interiors would be caused by
Saturn's strong gravitational pull as well as help from Dione and
Enceladus' orbital resonance; Enceladus completes two orbits of
Saturn for every one achieved by Dione.
Full story
here
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